Issue |
A&A
Volume 559, November 2013
|
|
---|---|---|
Article Number | A12 | |
Number of page(s) | 14 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201221012 | |
Published online | 29 October 2013 |
Online material
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Fig. 3
Abundance ratios [X/Fe] for aluminum and α-elements versus [Fe/H]. The data were taken from Luck & Heiter (2007) (black crosses); Reddy et al. (2006) (green crosses); Fulbright (2000) (red crosses); Gratton & Sneden (1991), and For & Sneden (2011) (blue crosses). CD-41°15048 and HD 214362 are represented by black squares. |
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Fig. 4
Abundance ratios [X/Fe] for the iron group elements versus [Fe/H]. Symbols have the same meaning as in Fig. 3. |
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Fig. 5
Abundance ratios [X/Fe] for the heavy elements. Symbols have the same meaning as in Fig. 3, except for zirconium and lanthanum. For zirconium we used the results of Edvardsson et al. (1993) (black crosses), and for lanthanum we used the results of Mishenina et al. (2006) (black crosses). |
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Fig. 8
Same as in Fig. 7, but in the YZ plane. |
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Fig. 10
Same as in Fig. 9, but in the YZ plane. |
Open with DEXTER |
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Fig. 11
Same as in Fig. 7, but for BD+09°3223 in the XY plane. The present position is labeled with “X”. |
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Fig. 12
Same as in Fig. 11, but in the YZ plane. |
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Observed Fe i and Fe ii lines.
Other lines studied.
Abundance uncertainties for CD-41°15048.
© ESO, 2013
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